Abstract
We study the impact of applying stochastic forcing to the Ghil-Sellers energy balance climate model in the form of a fluctuating solar irradiance. Through numerical simulations, we explore the noise-induced transitions between the competing warm and snowball climate states. We consider multiplicative stochastic forcing driven by Gaussian and α-stable Lévy – α ∈ (0, 2) – noise laws, and examine the statistics of transition times and most probable transition paths. While the Gaussian noise case – used here as a reference – has been extensively studied in a plethora of studies on metastable systems, much less is known about the Lévy case, both in terms of mathematical theory and heuristics, especially in the case of high- and infinite-dimensional systems. In the weak noise limit, the expected residence time in each metastable state scales in a fundamentally different way in the Gaussian vs. Lévy noise case with respect to the intensity of the noise. In the former case, the classical Kramers-like exponential law is recovered. In the latter case, power laws are found, with the exponent equal to −α, in apparent agreement with rigorous results obtained for additive noise in a related – yet different – reaction-diffusion equation as well as in simpler models. The transition paths are studied in a projection of the state space and remarkable differences are observed between the two different types of noise. The snowball-to-warm and the warm-to-snowball most probable transition path cross at the single unstable edge state on the basin boundary. In the case of Lévy noise, the most probable transition paths in the two directions are wholly separated, as transitions apparently take place via the closest basin boundary region to the outgoing attractor.
Highlights
1.1 Multistability of the Earth’s ClimateThe climate system comprises five interacting subdomains: the atmosphere, the hydrosphere, the upper layer of the lithosphere, the cryosphere, and the biosphere
We study the impact of applying stochastic forcing to the Ghil-Sellers energy balance climate model in the form of a fluctuating solar irradiance
It has become apparent that more general classes of α-stable Lévy noise laws might be suitable for modeling the observed climatic phenomena
Summary
1.1 Multistability of the Earth’s ClimateThe climate system comprises five interacting subdomains: the atmosphere, the hydrosphere (water in liquid form), the upper layer of the lithosphere, the cryosphere (water in solid form), and the biosphere (ecosystems and living organisms). The climate 20 is driven by the inhomogeneous absorption of incoming solar radiation, which sets up nonequilibrium conditions. In order to analyze the influence of random perturbations on the deterministic dynamics of the climate model described, we perturb the relative intensity μ of solar radiation by a symmetric α-stable Lévy process and rewrite Eq (1) in the form of the following stochastic partial differential equation (SPDE). With boundary and initial conditions defined by Eq (2) where T is the evolving stochastic temperature field. The research interest on this type of SPDEs (Løkka et al, 2004; Doering, 1987; Peszat and Zabczyk, 2007; Duan and Wang, 2014; Alharbi, 2021) is mainly focused on defining weak, strong, mild, and martingale solutions, and in specifying under which conditions these solutions exist and are unique, and in constructing numerical approximation schemes for the solutions (Davie and Gaines, 2000; Cialenco et al, 2012; Burrage and Lythe, 220 2014; Jentzen and Kloeden, 2009; Kloeden and Shott, 2001), among other aspects
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